Lecture 34 – The Milky Way Galaxy
Summary / Checklist of the Main Concepts to Understand and Remember

What is the Milky Way?  
How did our view of the Milky Way change after Galileo's observations in the 1600s?  
What is the concept of an "island universe", and when did we find out that there are other galaxies outside ours?  
How is the "Milky Way" that we see in the sky related to the Milky Way galaxy? How much of the galaxy are we seeing in the sky at night?  
Size and Structure  
What is the general shape of our galaxy, and what are the disk, bulge, and halo?  
What is the difference between the types of objects we find in the disk and in the halo of our galaxy?  
How wide is our galaxy, and approximately how many stars does it contain? How do we know those things?  
How do we know in what direction the center of our galaxy is? Why can't we use regular telescopes to look there, and What can we use?  
What is the object in the middle, How massive is it, and How do we know?  
In what part of the galaxy are we, and How far out from the center is our location?  
Evolution and Motion  
How did our galaxy form? (What is one important difference with respect to the way stars form?) How did it get to have this shape?  
Are stars being formed right now? In what part of the galaxy? Are stars in the disk and the halo made of exactly the same type of material?  
Approximately how fast do stars in our galaxy move? What is so puzzling about this fact?  
What do we think will be the eventual fate of our galaxy, billions of years from now?  
What is right outside our galaxy, and what evidence do we have that our galaxy may have absorbed smaller ones in the past?  

Topics from the lecture page and textbook not listed above [or between square brackets] were not covered in class;
Underlined words indicate that I will expect students to remember a number or a name related to that topic.

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